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astro-ph2000
Superconducting Superfluids in Neutron Stars
Brandon Carter
For treatment of the layers below the crust of a neutron star it is useful to employ a relativistic model involving three independently moving constituents, representing superfluid…
astro-ph2000
Centrifugal buoyancy as a mechanism for neutron star glitches
Brandon Carter, David Langlois, David M. Sedrakian
The frequent glitches (sudden increases of the apparent angular velocity) observed in certain pulsars are generally believed to be attributable to discontinuous angular momentum tr…